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High-mass star and massive cluster formation in the milky way
F Motte, S Bontemps, F Louvet - Annual Review of Astronomy …, 2018 - annualreviews.org
This review examines the state-of-the-art knowledge of high-mass star and massive cluster
formation, gained from ambitious observational surveys, which acknowledges the multiscale …
formation, gained from ambitious observational surveys, which acknowledges the multiscale …
Toward understanding massive star formation
H Zinnecker, HW Yorke - Annu. Rev. Astron. Astrophys., 2007 - annualreviews.org
Although fundamental for astrophysics, the processes that produce massive stars are not
well understood. Large distances, high extinction, and short timescales of critical …
well understood. Large distances, high extinction, and short timescales of critical …
A direct localization of a fast radio burst and its host
Fast radio bursts, are astronomical radio flashes of unknown physical nature with durations
of milliseconds. Their dispersive arrival times suggest an extragalactic origin and imply radio …
of milliseconds. Their dispersive arrival times suggest an extragalactic origin and imply radio …
The unWISE catalog: two billion infrared sources from five years of WISE imaging
EF Schlafly, AM Meisner… - The Astrophysical Journal …, 2019 - iopscience.iop.org
We present the unWISE Catalog, containing the positions and fluxes of roughly 2 billion
objects observed by the Wide-field Infrared Survey Explorer (WISE) over the full sky. The …
objects observed by the Wide-field Infrared Survey Explorer (WISE) over the full sky. The …
Chemical cartography with APOGEE: metallicity distribution functions and the chemical structure of the Milky Way disk
Using a sample of 69,919 red giants from the SDSS-III/APOGEE Data Release 12, we
measure the distribution of stars in the [α/Fe] versus [Fe/H] plane and the metallicity …
measure the distribution of stars in the [α/Fe] versus [Fe/H] plane and the metallicity …
ATLASGAL–properties of a complete sample of Galactic clumps
JS Urquhart, C König, A Giannetti… - Monthly Notices of …, 2018 - academic.oup.com
Abstract The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is an unbiased
870 μm submillimetre survey of the inner Galactic plane (| ℓ|< 60° with| b|< 1 5). It is the …
870 μm submillimetre survey of the inner Galactic plane (| ℓ|< 60° with| b|< 1 5). It is the …
Sloan digital sky survey IV: Map** the Milky Way, nearby galaxies, and the distant universe
MR Blanton, MA Bershady, B Abolfathi… - The Astronomical …, 2017 - iopscience.iop.org
The Sloan Digital Sky Survey (SDSS; York et al. 2000) started observations in 1998 and has
completed three different phases. The data collected includes optical imaging of most of the …
completed three different phases. The data collected includes optical imaging of most of the …
Cloud–cloud collisions and triggered star formation
Star formation is a fundamental process for galactic evolution. One issue over the last
several decades has been determining whether star formation is induced by external …
several decades has been determining whether star formation is induced by external …
Final targeting strategy for the SDSS-IV APOGEE-2S survey
APOGEE is a high-resolution (R∼ 22,000), near-infrared, multi-epoch, spectroscopic survey
of the Milky Way. The second generation of the APOGEE project, APOGEE-2, includes an …
of the Milky Way. The second generation of the APOGEE project, APOGEE-2, includes an …
ATLASGAL–The APEX telescope large area survey of the galaxy at 870 m
Context. Thanks to its excellent 5100 m high site in Chajnantor, the Atacama Pathfinder
Experiment (APEX) systematically explores the southern sky at submillimeter wavelengths …
Experiment (APEX) systematically explores the southern sky at submillimeter wavelengths …